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	Figure 4: CoRoT lightcurves of all candidates discussed in this paper: the light curve is phase-folded and the full orbital phase is shown. The iterative reconstruction filter (Alapini & Aigrain, subm.) is applied to the data, in order to correct for long-term instrumental and activity-related features while preserving the variation at the transit period.
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	Figure 5: CoRoT lightcurves of all candidates discussed in this paper (cont'd).
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	Figure 6: CoRoT lightcurves of all candidates discussed in this paper (cont'd). For single transits, the full light curve is shown against Julian Date.
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	Figure 7: CoRoT lightcurves of all candidates discussed in this paper (cont'd): zoom on the primary transits. The X-axis corresponds to the orbital phase when the period is determined, and Julian Date otherwise.
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Table 2:   Pre-launch information on IRa01 transit candidates derived from multi-colour photometry.

Table 3:   Radial-velocity measurements of E2-3854. SO stands for SOPHIE and HA for HARPS.

Table 4:   Radial-velocity measurements of 0102763847/E1-1158.

Table 5:   Radial-velocity measurements of E1-0399. CO stands for CORALIE at the Euler 120cm Swiss telescope.

Table 6:   Radial-velocity measurements of E2-3856.

Table 7:   Radial-velocity measurements of E2-2430.

Table 8:   Radial-velocity measurements of 0102855534/E1-1736.

Table 9:   Radial-velocity measurements of 0102855472/E2-0704.

Table 10:   Radial-velocity measurements of 0102798247/E2-1857.

Table 11:   Radial-velocity measurements of 0102788073/E2-2009.

Table 12:   Radial-velocity measurements of 0102869286/E1-2329.

Table 13:   Radial-velocity measurements of 0102876631/E1-3336.

Table 15:   Radial-velocity measurements of E1-4998.

Table 16:   Radial-velocity measurements of E2-3425.

Table 17:   Radial-velocity measurements of E1-4108.